|
|
Paper: |
Can the Propeller Outflow from AE Aquarii be Imaged Directly? |
Volume: |
315, Magnetic Cataclysmic Variables (IAU Colloquium 190) |
Page: |
293 |
Authors: |
Still, M.; Horne, K.; Knigge, C. |
Abstract: |
We calculate the Hα luminosity of an outflow nebula resulting from propeller action in AE Aqr. While the outflow is bright enough to be detected as an extended source, 1 arcsec across, it is dominated by the point-spread function (PSF) wings of the central object. By subtracting a PSF model from HST PC data we rule out the extreme models of high mass-loss rate combined with narrow-angle outflow, but more precise measurements are required to explore the propeller parameter space further. |
|
|
|
|